NAOC Open IR
Overview of the LAMOST-Kepler project
Fu, Jian-Ning1; De Cat, Peter2; Zong, Weikai1; Frasca, Antonio3; Gray, Richard O.4; Ren, An-Bin5; Molenda-Zakowicz, Joanna6; Corbally, Christopher J.7; Catanzaro, Giovanni3; Shi, Jian-Rong8; Luo, A-Li8; Zhang, Hao-Tong8
2020-10-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
ISSN1674-4527
Volume20Issue:10Pages:10
AbstractThe NASA Kepler mission obtained long-term high-quality photometric observations for a large number of stars in its original field of view from 2009 to 2013. To provide reliable stellar parameters in a homogeneous way, the LAMOST telescope began to carry out low-resolution spectroscopic observations for as many stars as possible in the Kepler field in 2012. By June 2018, 238 386 low-resolution spectra with SNRg >= 6 had been collected for 155 623 stars in the Kepler field, enabling the determination of atmospheric parameters and radial velocities, as well as spectral classification of the target stars. This information has been used by astronomers to carry out research in various fields, including stellar pulsations and asteroseismology, exoplanets, stellar magnetic activity and flares, peculiar stars and the Milky Way, binary stars, etc. We summarize the research progress in these fields where the usage of data from the LAMOST-Kepler (LK) project has played a role. In addition, time-domain medium-resolution spectroscopic observations have been carried out for about 12 000 stars in four central plates of the Kepler field since 2018. The currently available results show that the LAMOST-Kepler medium resolution (LK-MRS) observations provide qualified data suitable for research in additional science projects including binaries, high-amplitude pulsating stars, etc. As LAMOST is continuing to collect both low- and medium-resolution spectra of stars in the Kepler field, we expect more data to be released continuously and new scientific results to appear based on the LK project data.
Keywordastronomical database miscellaneous technique spectroscopy stars general stars statistics
Funding OrganizationNational Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation
DOI10.1088/1674-4527/20/10/167
WOS KeywordGIANT BRANCH STARS ; DATA RELEASE ; STELLAR ; PARAMETERS ; TELESCOPE ; ASTEROSEISMOLOGY ; GRANULATION ; BINARIES ; SYSTEM ; RICH
Language英语
Funding ProjectNational Development and Reform Commission ; National Natural Science Foundation of China (NSFC)[11833002] ; Beijing Natural Science Foundation[1194023]
Funding OrganizationNational Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation ; National Development and Reform Commission ; National Development and Reform Commission ; National Natural Science Foundation of China (NSFC) ; National Natural Science Foundation of China (NSFC) ; Beijing Natural Science Foundation ; Beijing Natural Science Foundation
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000587774600001
PublisherNATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/80893
Collection中国科学院国家天文台
Corresponding AuthorFu, Jian-Ning; Zong, Weikai
Affiliation1.Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China
2.Royal Observ Belgium, Ringlaan 3, B-1180 Brussels, Belgium
3.INAF Osservatorio Astrofis Catania, Via S Sofia 78, I-95123 Catania, Italy
4.Appalachian State Univ, Dept Phys & Astron, Boone, NC 28608 USA
5.China West Normal Univ, Dept Astron, Nanchong 637002, Peoples R China
6.Univ Wroclaw, Astron Inst, Ul Kopernika 11, PL-51622 Wroclaw, Poland
7.Univ Arizona, Vatican Observ Res Grp, Tucson, AZ 85721 USA
8.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100101, Peoples R China
Recommended Citation
GB/T 7714
Fu, Jian-Ning,De Cat, Peter,Zong, Weikai,et al. Overview of the LAMOST-Kepler project[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2020,20(10):10.
APA Fu, Jian-Ning.,De Cat, Peter.,Zong, Weikai.,Frasca, Antonio.,Gray, Richard O..,...&Zhang, Hao-Tong.(2020).Overview of the LAMOST-Kepler project.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,20(10),10.
MLA Fu, Jian-Ning,et al."Overview of the LAMOST-Kepler project".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 20.10(2020):10.
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